journal article·2024-03-06

Achieving Compatible p/n-Type Half-Heusler Compositions in Valence Balanced/Unbalanced Mg1–xVxNiSb

Kazuki Imasato, Hidetoshi Miyazaki, Philipp Sauerschnig, Kishor Kumar Johari, Takao Ishida, Atsushi Yamamoto, Michihiro Ohta

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Abstract

In thermoelectric and other inorganic materials research, the significance of half-Heusler (HH) compositions following the 18-electron rule has drawn interest in developing and exploiting the potential of intermetallic compounds. For the fabrication of thermoelectric modules, in addition to high-performance materials, having both p- and n-type materials with compatible thermal expansion coefficients is a prerequisite for module development. In this work, the p-type to n-type transition of valence balanced/unbalanced HH composition of Mg 1– x V x NiSb was demonstrated by changing the Mg:V chemical ratio. The Seebeck coefficient and power factor of Ti-doped Mg 0.57 V 0.33 Ti 0.1 NiSb are −130 μV K –1 and 0.4 mW m –1 K –2 at 400 K, respectively. In addition, the reduced lattice thermal conductivity (κ L < 2.5 W m –1 K –1 at 300 K) of n-type compositions was reported to be much smaller than κ L of conventional HH materials. As high thermal conductivity has long been an issue for HH materials, the synthesis of p- and n-type Mg 1– x V x NiSb compositions with low lattice thermal conductivity is a promising strategy for producing high-performance HH compounds. Achieving both p- and n-type materials from similar parent composition enabled us to fabricate a thermoelectric module with maximum output power P max ∼ 63 mW with a temperature difference of 390 K. This finding supports the benefit of exploring the huge compositional space of valence balanced/unbalanced quaternary HH compositions for further development of thermoelectric devices.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Heusler alloys: electronic and magnetic properties · Advanced Thermoelectric Materials and Devices · Magnetic and transport properties of perovskites and related materials

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

Affiliations

Global Zero Emission Research Center, National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba, Ibaraki 305-8569, Japan

Max Planck Institute for Chemical Physics of Solids, Dresden 01187, Germany

Department of Physical Science and Engineering, Nagoya Institute of Technology, Nagoya 466-8555, Japan

Funding

Japan Society for the Promotion of Science

References (47)

Show source-provided references
1. 10.1039/D1MA00707F10.1039/D1MA00707F ↗
2. 10.1016/j.progsolidstchem.2011.02.00110.1016/j.progsolidstchem.2011.02.001 ↗
3. 10.1088/2515-7655/ac49dc10.1088/2515-7655/ac49dc ↗
4. 10.3390/cryst1307115210.3390/cryst13071152 ↗
5. 10.1103/PhysRevB.59.861510.1103/PhysRevB.59.8615 ↗
6. 10.1016/S0925-8388(03)00547-410.1016/S0925-8388(03)00547-4 ↗
7. 10.1063/1.305638410.1063/1.3056384 ↗
8. 10.1016/j.actamat.2016.08.08010.1016/j.actamat.2016.08.080 ↗
9. 10.1002/advs.20190240910.1002/advs.201902409 ↗
10. 10.1002/adfm.20130066310.1002/adfm.201300663 ↗
11. 10.1016/j.actamat.2015.11.02210.1016/j.actamat.2015.11.022 ↗
12. 10.1016/j.actamat.2010.04.02810.1016/j.actamat.2010.04.028 ↗
13. 10.1021/acs.chemmater.6b0458310.1021/acs.chemmater.6b04583 ↗
14. 10.1039/c8ee00306h10.1039/c8ee00306h ↗
15. 10.1002/aenm.20180140910.1002/aenm.201801409 ↗
16. 10.1021/acs.jpcc.0c0068110.1021/acs.jpcc.0c00681 ↗
17. 10.1016/j.actamat.2016.01.03110.1016/j.actamat.2016.01.031 ↗
18. 10.1016/j.joule.2019.04.00310.1016/j.joule.2019.04.003 ↗
19. 10.1039/D2TA04593A10.1039/D2TA04593A ↗
20. 10.1002/adfm.20190504410.1002/adfm.201905044 ↗
21. 10.1002/aesr.20210020610.1002/aesr.202100206 ↗
22. 10.1002/pssa.20200009610.1002/pssa.202000096 ↗
23. 10.1038/2716710.1038/27167 ↗
24. 10.1002/advs.20230208610.1002/advs.202302086 ↗
25. 10.1016/j.materresbull.2023.11224610.1016/j.materresbull.2023.112246 ↗
26. 10.1021/acsaem.3c0025310.1021/acsaem.3c00253 ↗
27. 10.1016/j.jallcom.2022.16857210.1016/j.jallcom.2022.168572 ↗
28. 10.1021/acsami.0c1506310.1021/acsami.0c15063 ↗
29. 10.1016/j.joule.2017.11.00510.1016/j.joule.2017.11.005 ↗
30. 10.1039/C8CP04839H10.1039/C8CP04839H ↗
31. 10.1021/jacs.0c0706710.1021/jacs.0c07067 ↗
32. 10.1002/adma.20120291910.1002/adma.201202919 ↗
33. 10.1039/c9ta11328b10.1039/c9ta11328b ↗
34. 10.1063/1.490592210.1063/1.4905922 ↗
35. 10.1039/C7MH00865A10.1039/C7MH00865A ↗
36. 10.1103/PhysRevLett.84.367410.1103/PhysRevLett.84.3674 ↗
37. 10.1038/srep0688810.1038/srep06888 ↗
38. 10.1039/C4MH00142G10.1039/C4MH00142G ↗
39. 10.1063/1.495299410.1063/1.4952994 ↗
40. 10.1063/1.502109410.1063/1.5021094 ↗
41. 10.1002/adma.20200153710.1002/adma.202001537 ↗
42. 10.1039/D0TA08364J10.1039/D0TA08364J ↗
43. 10.1016/j.actamat.2017.03.07110.1016/j.actamat.2017.03.071 ↗
44. 10.1016/j.apenergy.2019.11444310.1016/j.apenergy.2019.114443 ↗
45. 10.1016/j.mtphys.2018.10.00110.1016/j.mtphys.2018.10.001 ↗
46. 10.1063/1.490824410.1063/1.4908244 ↗
47. 10.1063/1.514306110.1063/1.5143061 ↗